activity
19972007
most citedThe GLARE Survey II. Faint z=6 Ly-alpha Line Emitters in the HUDF

72 citations · 118 across the 4 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

7 papers · 2 filters

astro-ph2004

Multi-Object Near-IR H-alpha Spectroscopy of z~1 star-forming galaxies in the HDF-N

Michelle Doherty, Andrew Bunker, Robert Sharp +6

We present preliminary results from a programme to obtain multi-object near-infrared spectroscopy of galaxies at redshifts . We are using the instrument CIRPASS (the Cam…

astro-ph2004

CIRPASS: description, performance and astronomical results

Ian Parry, Andrew Bunker, Andrew Dean +9

The Cambridge Infra-red Panoramic Survey Spectrograph (CIRPASS) is described. This near-infrared (NIR) spectrograph has been used on the 8m Gemini-South Telescope, the 3.9m Anglo-A…

astro-ph2004

A Matched Catalogue i-dropout galaxies at z~6 in the Hubble Ultra Deep Field

Andrew J Bunker, Elizabeth R. Stanway

A recent preprint by Yan & Windhorst (astro-ph/0407493) independently repeats our selection of candidate z~6 galaxies in the Hubble Ultra Deep Field (astro-ph/0403223). The agreeme…

astro-ph2004

Star Formation at Redshift One: Preliminary results from an H-alpha Survey

M. Doherty, A. Bunker, R. Sharp +5

We present the first successful demonstration of multi-object near-infrared spectroscopy on high redshift galaxies. Our objective is to address the true star formation history of t…

astro-ph2004

Near-Infrared Properties of I-Drop Galaxies in the Hubble Ultra Deep Field

Elizabeth Stanway, Richard McMahon, Andrew Bunker

We analyse near-infrared HST/NICMOS F110W (J) and F160W (H) band photometry of a sample of 27 i'-drop candidate z~6 galaxies in the central region of the HST/ACS Ultra Deep Field (…

astro-ph2004

The Star Formation Rate of the Universe at z~6 from the Hubble Ultra Deep Field

A. J. Bunker, E. R. Stanway, R. S. Ellis +1

We determine the abundance of i'-band drop-outs in the recently-released HST/ACS Hubble Ultra Deep Field (UDF). Since the majority of these sources are likely to be z~6 galaxies wh…